Comet 210P/Christensen passes perihelion

Dominic Ford, Editor
From the Comets feed


Comet 210P/Christensen will make its closest approach to the Sun on 1 December, at a distance of 0.52 AU.

From Cambridge on the day of perihelion it will not be readily observable since it will be very close to the Sun, at a separation of only 10° from it.

The events that comprise the 1980 apparition of 210P/Christensen are as follows:

Date Event
01 Dec 1980Comet 210P/Christensen passes perihelion

The table below lists the times when 210P/Christensen will be visible from Cambridge day-by-day through its apparition:

Date Constellation Comet visibility
10 Nov 1980SagittariusNot observable
12 Nov 1980SagittariusNot observable
14 Nov 1980ScorpiusNot observable
16 Nov 1980ScorpiusNot observable
18 Nov 1980ScorpiusNot observable
20 Nov 1980ScorpiusNot observable
22 Nov 1980ScorpiusNot observable
24 Nov 1980ScorpiusNot observable
26 Nov 1980ScorpiusNot observable
28 Nov 1980ScorpiusNot observable
30 Nov 1980ScorpiusNot observable
02 Dec 1980ScorpiusNot observable
04 Dec 1980ScorpiusNot observable
06 Dec 1980LibraNot observable
08 Dec 1980LibraNot observable
10 Dec 1980LibraNot observable
12 Dec 1980LibraNot observable
14 Dec 1980LibraNot observable
16 Dec 1980LibraNot observable
18 Dec 1980LibraNot observable
20 Dec 1980LibraNot observable

A more detailed table of 210P/Christensen's position on each night is available here. A diagram of the orbit of 210P/Christensen is available here.

Finder chart

The chart below shows the path of 210P/Christensen over the course of its apparition, as calculated from the orbital elements published by the Minor Planet Center (MPC). It is available for download, either on dark background, in PNG, PDF or SVG formats, or on a light background, in PNG, PDF or SVG formats. It was produced using StarCharter.

Comet brightnesses

Comets are intrinsically highly unpredictable objects, since their brightness depends on the scattering of sunlight from dust particles in the comet's coma and tail. This dust is continually streaming away from the comet's nucleus, and its density at any particular time is governed by the rate of sublimation of the ice in the comet's nucleus, as it is heated by the Sun's rays. It also depends on the amount of dust that is mixed in with that ice. This is very difficult to predict in advance, and can be highly variable even between successive apparitions of the same comet.

In consequence, while the future positions of comets are usually known with a high degree of confidence, their future brightnesses are not. For most comets, we do not publish any magnitude estimates at all. For the few comets where we do make estimates, we generally prefer the BAA's magnitude parameters to those published by the Minor Planet Center, since they are typically updated more often.

No estimate for the brightness of comet 210P/Christensen is currently available.

The comet's position at perihelion will be:

Object Right Ascension Declination Constellation Magnitude
Comet 210P/Christensen 15h46m10s 22°52'S Libra 9.8

The coordinates are given in J2000.0.

The sky on 23 Nov 2024

The sky on 23 November 2024
Sunrise
06:43
Sunset
16:15
Twilight ends
17:54
Twilight begins
05:03


Waning Crescent

36%

22 days old

Planets
Rise Culm. Set
Mercury 08:33 12:55 17:17
Venus 10:09 14:32 18:54
Moon 23:09 06:06 12:50
Mars 20:36 04:03 11:30
Jupiter 17:09 00:40 08:11
Saturn 12:58 18:29 23:59
All times shown in EST.

Warning

Never attempt to point a pair of binoculars or a telescope at an object close to the Sun. Doing so may result in immediate and permanent blindness.

Source

This event was automatically generated on the basis of orbital elements published by the Minor Planet Center (MPC) , and is updated whenever new elements become available. It was last updated on 13 Oct 2024.

Image credit

© Andy Roberts 1997. Pictured comet is C/1995 O1 Hale-Bopp.

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